New Evidence Supports the Existence of the Elusive Planet Nine

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Found
beyond the orbit of Neptune, the Kuiper Belt is the most distant area in our solar
system, and it’s home to the now six known dwarf planets (including Pluto) and
other cosmic objects. It could also be the home of our system’s rogue ninth
planet, the (un)imaginatively titled Planet Nine.

Researchers
from the University of Arizona (UA) have weighed in on the search for this
phantom planet in a new study published in Astrophysical
Journal Letters. Led by Regents’ Professor of Planetary Sciences Renu
Malhotra, the team at UA’s Lunar and Planetary Lab found that the orbital
behaviors of some Kuiper Belt objects (KBO) could likely be explained by the
presence of Planet Nine.

KBOs
are typically influenced by the gravity of the four big planets in our solar
system, but not so for four of the most distant KBOs. These extreme KBOs, or
eKBOs, show large orbital eccentricities, getting close to the Sun at one point
and swinging farther out at another.

“We
analyzed the data of these most distant Kuiper Belt objects and noticed
something peculiar, suggesting they were in some kind of resonances with an
unseen planet,” Malhotra explains.

Furthermore,
the orbital period ratios of these eKBOs are small whole numbers, suggesting an
elliptical orbit that only the presence of a massive planet could stabilize,
one the researchers estimate has roughly ten times the mass of Earth.

Known
KBOs. Credits: Wikipedia/CC BY-SA 3.0

EXPANDING
OUR HORIZONS

The
results of the UA study were presented at the joint 48th meeting of the
Division for Planetary Sciences of the American Astronomical Society and 11th
European Planetary Science Congress in Pasadena, California this
week. While Malhotra believes their paper provides valuable information
about the hypothetical Planet Nine, they are aware that they haven’t
definitively proven its existence just yet.

Despite
the many observed Kuiper Belt occurrences and computer models that suggests
Planet Nine exists, until someone actually sees it, we can’t be sure it’s
there, but we might not have to wait too much longer for
confirmation. Over the next few years, our capacity to see our galactic
surroundings will significantly improve with the launch of better space telescopes, including the James Webb Space Telescope (JWST), which is expected
to be ready for use in 2018. Until then, evidence like that uncovered in the UA
study can tell us a lot about the unseen corners of our solar system.